Spectral line Variations of the Symbiotic Variable CH Cygni

  • Yoo Kye Hwa (Department of Science Education, Ewha Womans University) ;
  • Kim Kang Min (Korea Astronomy Observatory) ;
  • Lee Byung Chul (Korea Astronomy Observatory) ;
  • Yoon Tae Seog (Department of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • Lee Jung Ae (Department of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • Kang Yong Hee (Department of Earth Science Education, Kyungpook National University)
  • Published : 2005.03.01

Abstract

A series of high resolution spectra of CH Cygni obtained at the Bohyunsan Optical Astronomy Observatory (BOAO) in April 2004 has been analyzed. The emission components of the [O I] 6300 A lines are de-convoluted and fitted with Gaussian functions in order to investigate the characteristics and the structure of CH Cygni system along with the analysis for $H{\alpha}$ and [O III] lines. A present geometrical structure of the components of CH Cygni system is suggested.

Keywords

References

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